A GLIMPSE AT QUASAR HOST GALAXY FAR-UV EMISSION USING DAMPED Ly alpha%26apos;s AS NATURAL CORONAGRAPHS

作者:Cai Zheng*; Fan Xiaohui; Noterdaeme Pasquier; Wang Ran; McGreer Ian; Carithers Bill; Bian Fuyan; Miralda Escude Jordi; Finley Hayley; Paris Isabelle; Schneider Donald P; Zakamska Nadia L; Ge Jian; Petitjean Patrick; Slosar Anze
来源:Astrophysical Journal, 2014, 793(2): 139.
DOI:10.1088/0004-637X/793/2/139

摘要

In merger-driven models of massive galaxy evolution, the luminous quasar phase is expected to be accompanied by vigorous star formation in quasar host galaxies. In this paper, we use high column density damped Ly alpha (DLA) systems along quasar sight lines as natural coronagraphs to directly study the far-UV (FUV) radiation from the host galaxies of luminous background quasars. We have stacked the spectra of similar to 2000 DLA systems (N-H (I) %26gt; 10(20.6) cm(-2)) with a median absorption redshift %26lt; z %26gt; = 2.6 selected from quasars observed in the SDSS-III Baryon Oscillation Spectroscopic Survey. We detect residual flux in the dark troughs of the composite DLA spectra. The level of this residual flux significantly exceeds systematic errors in the Sloan Digital Sky Survey fiber sky subtraction; furthermore, the residual flux is strongly correlated with the continuum luminosity of the background quasar, while uncorrelated with DLA column density or metallicity. We conclude that the flux could be associated with the average FUV radiation from the background quasar host galaxies (with medium redshift %26lt; z %26gt; = 3.1) that is not blocked by the intervening DLA. Assuming that all of the detected flux originates from quasar hosts, for the highest quasar luminosity bin (%26lt; L %26gt; = 2.5 x 10(13) L-circle dot), the host galaxy has an FUV intensity of 1.5 +/- 0.2 x 10(40) erg s(-1) angstrom(-1); this corresponds to an unobscured UV star formation rate of 9 M-circle dot yr(-1).

  • 出版日期2014-10-1